EAS Publications Series
Volume 36, 2009Dark Energy and Dark Matter: Observations, Experiments and Theories
|Page(s)||231 - 236|
|Published online||30 May 2009|
E. Pécontal, T. Buchert, Ph. Di Stefano and Y. Copin (eds)
EAS Publications Series, 36 (2009) 231-236
Max-Planck-Institut für Physik, Föhringer Ring 6,
80805 München, Germany
2 Eberhard-Karls-Universität Tübingen, 72076 Tübingen, Germany
3 On leave from: Departamento de Fisica, Universidade de Coimbra, 3004 516 Coimbra, Portugal
4 Department of Physics, University of Oxford, Oxford OX1 3RH, UK
5 INFN, Laboratori Nazionali del Gran Sasso, 67010 Assergi, Italy
6 Physik-Department E15, Technische Universität München, 85747 Garching, Germany
7 Now at: Department of Physics, Queen's University, Ontario K7L 3N6, Canada
The CRESST-II direct Dark Matter search is located in the Gran Sasso underground laboratories, Italy. CaWO4 crystals are used as scintillating targets for WIMP (weakly interacting massive particle) interactions. They are operated as cryogenic calorimeters in combination with a second cryogenic detector used to measure the scintillation light produced in the target crystal. For each particle interaction, the combination of phonon and light signals provides an event by event discrimination which allows to distinguish known particles (alphas, betas, gammas, neutrons) from the expected signal of WIMPs. A major upgrade of the setup comprises modifications of the shielding, installation of a muon-veto, and new read out electronics, as well as a new detector-support structure to accommodate up to 33 detector modules, i.e. 10 kg of target mass. The experiment was thereafter successfully commissioned in 2007. Data obtained during this commissioning phase from 2 detector modules are presented here. Combining the data collected with these two detector modules with data from one single module obtained during the CRESST-I phase, the experiment could already place a limit of ~6 × 10-7 pb for the spin independent WIMP-nucleon scattering cross section at a WIMP mass of ~60 GeV/c2.
© EAS, EDP Sciences, 2009
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